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Mira (ο Ceti, 68 Ceti) je dvojhvězdný systém v souhvězdí Velryby, tvořený pulzujícím červeným obrem Mira A a horkým bílým trpaslíkem Mira B. Druhá složka zachycuje část látky odnášené hvězdným větrem hlavní hvězdy, a soustava se proto řadí mezi symbiotické dvojhvězdy.
The analysis highlights Historie pozorování a název, Mira A and Ztráta hmoty a ultrafialový chvost as prominent areas in the source structure around Mira.
Source areas are shown by the number of related topics found in each part of the analysis. Use smaller areas too: they can reveal specialized angles and content gaps.
Smaller areas are not necessarily less important. They contain fewer connections in this analysis and can be useful for finding specialized angles or coverage gaps.
High-confidence facts extracted from structured source data. Use them as anchors for further research.
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Browse the complete topic structure, not only the most central items. Less prominent entities and concepts can reveal missing angles, specialized context and useful research gaps. Each item opens a new analysis centered on that subject.
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The extracted context around Mira shows recurring relationship patterns in the source. For example, Mira → Aitken, ALMA, DA, Hubbleovým, Hubbleův, Jako, Joy, Miry, Pozorování, Průvodce, Snímky, VZ Ceti Another extracted example is Mira → David Fabricius, Fabricius, Historiola Mirae Stellae, Ismail Bouillaud, Johannes Hevelius, Johannes Phocylides Holwarda, Jupiterem, Merkur, Proměnnost Miry, Znovu. Use these groups to spot repeated connection types before inspecting the individual relationships.
Use these terms to understand the vocabulary surrounding the topic, not as a checklist for keyword stuffing.
přibližně let miry pozorování roku ceti 10 roce tedy mění soustava vlastní poloměr 68 mirid vzdálenost jako slunce hvězdu látky
TTTA extracted 79 structured relationships around Mira. Examples in this analysis include Mira → 2MASS → 2MASS J02192081-0258393 and Mira → Argument šířky pericentra → 212,6+6,2−21,0°. The table shows each extracted connection, where it came from and its confidence.
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Mira | 2MASS | 2MASS J02192081-0258393 | 1.00 | infobox |
| Mira | Argument šířky pericentra | 212,6+6,2−21,0° | 1.00 | infobox |
| Mira | Bayerovo označení | ο Cet | 1.00 | infobox |
| Mira | Bonner Durchmusterung | BD −03° 353 | 1.00 | infobox |
| Mira | Bright Star katalog | HR 681 | 1.00 | infobox |
| Mira | Deklinace | −02° 58′ 39,4956″ | 1.00 | infobox |
| Mira | Doba oběhu | 276,5+48,2−8,5 roku | 1.00 | infobox |
| Mira | Délka vzestupného uzlu | 149,9+3,5−9,5° | 1.00 | infobox |
| Mira | Excentricita dráhy | 0,665+0,041−0,140 | 1.00 | infobox |
| Mira | Flamsteedovo označení | 68 Cet | 1.00 | infobox |
| Mira | General Catalogue | GC 2796 | 1.00 | infobox |
| Mira | Henry Draper Catalogue | HD 14386 | 1.00 | infobox |
| Mira | Hmotnost | přibližně 1 M☉ | 1.00 | infobox |
| Mira | Hmotnost | 0,24 ± 0,04 nebo 0,42 ± 0,04 podle modelu akrece M☉ | 1.00 | infobox |
| Mira | Katalog Hipparcos | HIP 10826 | 1.00 | infobox |
| Mira | Katalog Tycho | TYC 4693-1144-1 | 1.00 | infobox |
| Mira | Oscilační perioda | 331,3 dne | 1.00 | infobox |
| Mira | Paralaxa | 10,91 ± 1,22 mas | 1.00 | infobox |
| Mira | Poloměr | 332–402 R☉ | 1.00 | infobox |
| Mira | Poloměr | přibližně 0,020 nebo 0,015 R☉ | 1.00 | infobox |
| Mira | Povrchová teplota | 2 918–3 192 K | 1.00 | infobox |
| Mira | Povrchová teplota | přibližně 14 000 K | 1.00 | infobox |
| Mira | Primární hvězda | Mira A | 1.00 | infobox |
| Mira | Průvodce | Mira B | 1.00 | infobox |
| Mira | Radiální rychlost | +63,50 ± 0,60 km/s | 1.00 | infobox |
| Mira | Rektascenze | 02h 19m 20,79210s | 1.00 | infobox |
| Mira | SAO katalog | SAO 129825 | 1.00 | infobox |
| Mira | SIMBAD | data (Mira A a systém) | 1.00 | infobox |
| Mira | SIMBAD | data (Mira B) | 1.00 | infobox |
| Mira | Sklon dráhy | 126,6+0,4−0,9° | 1.00 | infobox |
The concept neighborhoods around Mira bring nearby vocabulary together. In this analysis, examples include Souhvězdí, Systém and Dr3. Use the clusters to find adjacent concepts and terminology that may deserve separate research.
For Mira, one of the stronger structural bridges in this analysis connects Mira with Overview. Bridges highlight paths between different parts of the map and can reveal research angles that are easy to miss in a flat list.
TTTA analyzes the structure around Mira to surface related topics, entities, relationships, concept neighborhoods and bridge connections. Use the map to explore areas such as Historie pozorování a název, Mira A & Ztráta hmoty a ultrafialový chvost, including less central topics that may reveal useful research gaps. Automatically extracted connections are research leads rather than rewritten encyclopedia content.
Source: Wikipedia — Mira · CS edition · Analysis: TopicsToTalkAbout
